A compact, large-range interferometer for precision measurement and inertial sensing

Sam Cooper; Anna Green; Chris Collins; David Hoyland; Clive Speake; Andreas Freise; Conor Mow-Lowry

doi:10.1088/1361-6382/aab2e9

A compact, large-range interferometer for precision measurement and inertial sensing

Sam Cooper, Anna Green, Chris Collins, David Hoyland, Clive Speake, Andreas Freise, Conor Mow-Lowry

Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

7 Citations (Scopus)

174 Downloads (Pure)

Abstract

We present a compact, fibre-coupled interferometer with high sensitivity and a large working range. We propose to use this interferometer as a readout mechanism for future inertial sensors, removing a major limiting noise source, and in precision positioning systems. The interferometers peak sensitivity is 2 x 10^-14m/√Hz at 70 Hz and 8 x 10^-11m/√Hz at 10 mHz. If deployed on a GS-13 geophone, the resulting inertial sensing output will be dominated by suspension thermal noise from 50 mHz to 2 Hz.

Original language	English
Pages (from-to)	1-6
Journal	Classical and Quantum Gravity
Volume	35
Issue number	9
DOIs	https://doi.org/10.1088/1361-6382/aab2e9
Publication status	Published - 22 Mar 2018

Keywords

astro-ph.IM
physics.ins-det
optical interferometry
homodyne detection
optomechanics

Access to Document

10.1088/1361-6382/aab2e9Licence: None: All rights reserved

Cooper_et_al_A_compact_large-range_interferometer_for_precision_measurement_Classical_and_Quantum_Gravity_2018
This is an author-created, un-copyedited version of an article accepted for publication/published in Classical and Quantum Gravity. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at https://doi.org/10.1088/1361-6382/aab2e9
Accepted author manuscript, 1.17 MBLicence: Other (please specify with Rights Statement)

https://iopscience.iop.org/article/10.1088/1361-6382/aab2e9Licence: None: All rights reserved

Cite this

@article{1aacbf7d4aa04b85bd7f7eee50592478,

title = "A compact, large-range interferometer for precision measurement and inertial sensing",

abstract = "We present a compact, fibre-coupled interferometer with high sensitivity and a large working range. We propose to use this interferometer as a readout mechanism for future inertial sensors, removing a major limiting noise source, and in precision positioning systems. The interferometers peak sensitivity is 2 x 10-14 m/√Hz at 70 Hz and 8 x 10-11 m/√Hz at 10 mHz. If deployed on a GS-13 geophone, the resulting inertial sensing output will be dominated by suspension thermal noise from 50 mHz to 2 Hz.",

keywords = "astro-ph.IM, physics.ins-det, optical interferometry, homodyne detection, optomechanics",

author = "Sam Cooper and Anna Green and Chris Collins and David Hoyland and Clive Speake and Andreas Freise and Conor Mow-Lowry",

year = "2018",

month = mar,

day = "22",

doi = "10.1088/1361-6382/aab2e9",

language = "English",

volume = "35",

pages = "1--6",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing",

number = "9",

}

TY - JOUR

T1 - A compact, large-range interferometer for precision measurement and inertial sensing

AU - Cooper, Sam

AU - Green, Anna

AU - Collins, Chris

AU - Hoyland, David

AU - Speake, Clive

AU - Freise, Andreas

AU - Mow-Lowry, Conor

PY - 2018/3/22

Y1 - 2018/3/22

N2 - We present a compact, fibre-coupled interferometer with high sensitivity and a large working range. We propose to use this interferometer as a readout mechanism for future inertial sensors, removing a major limiting noise source, and in precision positioning systems. The interferometers peak sensitivity is 2 x 10-14 m/√Hz at 70 Hz and 8 x 10-11 m/√Hz at 10 mHz. If deployed on a GS-13 geophone, the resulting inertial sensing output will be dominated by suspension thermal noise from 50 mHz to 2 Hz.

AB - We present a compact, fibre-coupled interferometer with high sensitivity and a large working range. We propose to use this interferometer as a readout mechanism for future inertial sensors, removing a major limiting noise source, and in precision positioning systems. The interferometers peak sensitivity is 2 x 10-14 m/√Hz at 70 Hz and 8 x 10-11 m/√Hz at 10 mHz. If deployed on a GS-13 geophone, the resulting inertial sensing output will be dominated by suspension thermal noise from 50 mHz to 2 Hz.

KW - astro-ph.IM

KW - physics.ins-det

KW - optical interferometry

KW - homodyne detection

KW - optomechanics

U2 - 10.1088/1361-6382/aab2e9

DO - 10.1088/1361-6382/aab2e9

M3 - Article

SN - 0264-9381

VL - 35

SP - 1

EP - 6

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 9

ER -

A compact, large-range interferometer for precision measurement and inertial sensing

Abstract

Keywords

Access to Document

Fingerprint

Cite this